Залежність константи рівноваги від температури

Before this, knowВільна енергія Гіббса та рівновага

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Previously, we studied how Gibbs free energy relates to the equilibrium constant. But, we know that Gibbs free energy is temperature-dependent. So, we expect that the equilibrium constant is also temperature-dependent. Last time, we derived the formula, lnKeq=−ΔGoRTln{K_{eq}}=\frac{-\Delta G^{o}}{RT}. We used the formula to relate ΔG\Delta G and the equilibrium constant's magnitude. Now we can use it to study how temperature affects equilibrium.

The Van't Hoff Equation

We want to relate the equilibrium constant and temperature. But first, we need to derive the Van't Hoff equation. We'll start with the equation we found last time.

  1. lnKeq=−ΔGoRTln{K_{eq}}=\frac{-\Delta G^{o}}{RT}

  2. We know that ΔGo=ΔHo−TΔSo\Delta G^{o}=\Delta H^{o}-T\Delta S^{o}. Let's start by replacing ΔGo\Delta G^{o}. So, lnKeq=−ΔHoRT+ΔSoRln{K_{eq}}= \frac{-\Delta H^{o}}{RT}+\frac{\Delta S^{o}}{R}.

  3. Now we can do something strange. Let's subtract two equilibrium constants lnK1ln{K_{1}} at T1T_{1} and lnK2ln{K_{2}} at T2T_{2}. They are for the same reaction but at different temperatures. We can assume that the standard enthalpy change and standard entropy change are temperature-independent. So, lnK2−lnK1=(−ΔHoRT2+ΔSoR)−(−ΔHoRT1+ΔSoR)ln{K_{2}}-ln{K_{1}}=(\frac{-\Delta H^{o}}{RT_{2}}+\frac{\Delta S^{o}}{R})-(\frac{-\Delta H^{o}}{RT_{1}}+\frac{\Delta S^{o}}{R}).

  4. Now we can apply the rule of natural logs. We know that ln(x)−ln(y)=lnxyln{(x)}-ln{(y)}=ln{\frac{x}{y}}. So, lnK2−lnK1=lnK2K1ln{K_{2}}-ln{K_{1}}=ln{\frac{K_{2}}{K_{1}}}.

  5. We can also simplify the other side of the equation. (−ΔHoRT2+ΔSoR)−(−ΔHoRT1+ΔSoR)→−ΔHoRT2−−ΔHoRT1+ΔSoR−ΔSoR→ΔHoR×(1T1−1T2)(\frac{-\Delta H^{o}}{RT_{2}}+\frac{\Delta S^{o}}{R})-(\frac{-\Delta H^{o}}{RT_{1}}+\frac{\Delta S^{o}}{R})\rightarrow \frac{-\Delta H^{o}}{RT_{2}} -\frac{-\Delta H^{o}}{RT_{1}} + \frac{\Delta S^{o}}{R}-\frac{\Delta S^{o}}{R}\rightarrow \frac{\Delta H^{o}}{R}\times(\frac{1}{T_{1}}-\frac{1}{T_{2}}).

  6. So, we derived the Van't Hoff equation, lnK2K1=ΔHoR×(1T1−1T2)ln{\frac{K_{2}}{K_{1}}}=\frac{\Delta H^{o}}{R}\times(\frac{1}{T_{1}}-\frac{1}{T_{2}}).

Van't Hoff Plots

Let's return to the second step in our derivation. lnKeq=−ΔHoRT+ΔSoRln{K_{eq}}= \frac{-\Delta H^{o}}{RT}+\frac{\Delta S^{o}}{R}. The equation has the form y=mx+by=mx+b.

  • y=Keqy=K_{eq}
  • m=−HoRm=-\frac{H^{o}}{R}
  • x=1Tx=\frac{1}{T}
  • b=ΔSoRb=\frac{\Delta S^{o}}{R}

So, if we plot KeqK_{eq} against 1T\frac{1}{T}, we get a linear graph.

KeqK_{eq} and Enthalpy

What happens when are reactions are endothermic or exothermic? We can plug in the enthalpy change into Van't Hoff plot equation.

Endothermic

  • ΔH=+\Delta H= +

  • The slope is negative. So as 1T\frac{1}{T} increases, KeqK_{eq} decreases. As the temperature increases, KeqK_{eq} gets larger.

Exothermic

  • ΔH=−\Delta H= -

  • The slope is positive. So as 1T\frac{1}{T} increases, KeqK_{eq} increases. As the temperature increases, KeqK_{eq} gets smaller.

Using the Van't Hoff Equation

Let's use the Van't Hoff equation to confirm our conclusions.

Let's start with a generic endothermic reaction. At 25oC25^{o}C its Keq=0.00045K_{eq}=0.00045 and ΔH=15.0Jmol\Delta H=15.0\frac{J}{mol}. What is its KeqK_{eq} at 32oC32^{o}C?

  • Remember, this is an endothermic reaction. So, we expect KeqK_{eq} to increase.

  • lnK2K1=ΔHoR(1T1−1T2)→lnK20.00045=15.0Jmol8.314JmolK(1298.15K−1305.15K)→lnK20.00045=1.80→K2=0.0027ln\frac{K_{2}}{K_{1}}=\frac{\Delta H^{o}}{R}(\frac{1}{T_{1}}-\frac{1}{T_{2}})\rightarrow ln\frac{K_{2}}{0.00045}= \frac{15.0\frac{J}{mol}}{8.314\frac{J}{molK}}(\frac{1}{298.15K}-\frac{1}{305.15K}) \rightarrow ln\frac{K_{2}}{0.00045}=1.80 \rightarrow K_{2}=0.0027

  • K2>K1K_{2}>K_{1} like we expected.

Now, let's say we have a very exothermic reaction. At 25oC25^{o}C its Keq=0.00045K_{eq}=0.00045 and ΔH=−50,000.0Jmol\Delta H=-50,000.0\frac{J}{mol}. What is its KeqK_{eq} at 32oC32^{o}C?

  • For an exothermic reaction, we expect KeqK_{eq} to decrease.

  • lnK2K1=ΔHoR(1T1−1T2)→lnK20.00045=−50000.0Jmol8.314JmolK(.0000771K)→lnK20.00045=.097→K2=0.000044ln\frac{K_{2}}{K_{1}}=\frac{\Delta H^{o}}{R}(\frac{1}{T_{1}}-\frac{1}{T_{2}}) \rightarrow ln\frac{K_{2}}{0.00045}=\frac{-50000.0\frac{J}{mol}}{8.314\frac{J}{molK}}(.000077\frac{1}{K})\rightarrow ln\frac{K_{2}}{0.00045}=.097 \rightarrow K_{2}=0.000044

  • K2<K1K_{2}<K_{1}, like we expected.

We used the Van't Hoff equation to confirm our conclusion!

Video

(Video) Free Energy, Equilibrium Constants and Temperature

Webcast-legacy Departmental

This quick video will show you the relationship between the equilibrium constant and temperature. The video starts by connecting the Gibbs free energy to the equilibrium constant. Then, they display the graphs of K vs. T and ln[(K)]ln[(K)] vs. 1T\frac{1}{T}. So, you get to visualize the relationship between equilibrium constants and temperatures.

Type a concept, like “slope” or “photosynthesis”.

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